A Computational Study of Molecular Conformers Jordan Haskins Andrew Fleming Amanda Petty Gino Moore
Introduction As bonds rotate, changing a molecules conformation from anti to staggered to eclipsed, the energy associated with the atoms composing that molecule changes. The purpose of this experiment is to measure the change in energy and the shielding constants for each of the hydrogen and carbon atoms in 1,2-dichloroethane.
Materials and Methods In this experiment we used Gaussian 98
to compute the energies of four different conformers of 1,2dichloroethane. These energies were then compared to the expected energies. Using Gaussian 98, we calculated the chemical shifts of the hydrogens and carbons in the conformers. Next we compared the predicted chemical shifts to the known chemical shifts given in literature.
Materials and Methods We used Microsoft Excel to perform the
calculations. Instructions for the experiment were given in a handout from Dr. Howard. Recorded energies for each conformer, along
with its isotopic shielding constant, for hydrogen and carbon where obtained from Gaussian 98.
Materials and Methods The shielding constants are: 31.8835ppm for hydrogen 187.3250ppm for carbon
Results Conformer
Calculated shielding constant (σ, ppm)
Calculated chemical shift (δcalc, ppm)
Anti
28.4778
3.4057
Staggered (hydrogens 1,2)
28.2945
3.5890
Staggered (hydrogens 3,4)
28.2340
3.6495
Eclipsed 1
28.3056
3.5779
Eclipsed 2 (Hydrogens 1,2)
28.3749
3.5086
Eclipsed 2 (Hydrogen 3,4)
27.9314
3.9521
Results Conformer
Calculated shielding constant (σ, ppm)
Calculated chemical shift (δcalc, ppm)
Anti
138.0219
49.3031
Staggered
133.2141
54.1109
Eclipsed 1
140.2585
47.0665
Eclipsed 2
133.7496
53.5754
Results The experimental chemical shifts of 1,2 dichloroethane were:
Hydrogen
Carbon
3.729 ppm
43.60 ppm
These values were given in the Spectral Database System.
Results Conformer
Calculated Experimental Chemical shift Chemical shift (δcalc ) (δexp)
Percent Error (%)
Anti
3.4057 ppm
3.729 ppm
8.67
Staggered (Hydrogens 1,2)
3.5890 ppm
3.729 ppm
3.75
Staggered (Hydrogens 3,4)
3.6495 ppm
3.729 ppm
2.13
Eclipsed 1
3.5779 ppm
3.729 ppm
4.05
Eclipsed 2 (Hydrogens 1,2)
3.5086 ppm
3.729 ppm
5.91
Eclipsed 2 (Hydrogens 3,4)
3.9521 ppm
3.729 ppm
5.98
Results Conformer
Calculated Chemical shift (δcalc )
Experimental Chemical shift (δexp)
Percent Error (%)
Anti
49.3031 ppm
43.60 ppm
13.1
Staggered
54.1109 ppm
43.60 ppm
24.1
Eclipsed 1
47.0665 ppm
43.60 ppm
8.0
Eclipsed 2
53.5754 ppm
43.60 ppm
22.9
Results Conformer
Energy (Hartrees)
Anti
-1000.04022175
Staggered
-1000.03796939
Eclipsed 1
-1000.02614119
Eclipsed 2
-1000.03303489
Discussion Based on our calculations, we found that
the anti conformer was the most stable. This is due to the fact that it is where the largest electron clouds are the farthest apart. Also, the eclisped conformer in which the chlorines overlap was the least stable. This is due to the largest electron clouds being in closest proximity.
Discussion Since rotation is rapid around the C-C
double bond, the NMR instrument recognizes only an “average” molecule. So, the chemical shifts are an average of the different conformers. Gaussian gave chemical shifts that were different than the reported experimental values: the carbon chemical shifts were too high the hydrogen chemical shifts were too low
This is due to Gaussian underestimating
the electron density near the nucleus if the chemical shift is too high and overestimating the electron density if the
Conclusion Since the model system used consisted only
of a single, motionless, gas-phase molecule, the setup wasn’t realistic. This could be remedied by having more molecules in the system so that there would be more molecular interactions. This may influence more accurate chemical shifts.
Citations Handout: A Computational Study of Molecular Conformers Spectral Database System.
http://www.aist.go.jp/RIODB/SDBS/menu-e.html Fleming, A.J.; Physical Chemistry Laboratory Notebook, 2007 p. 17-18. Haskins, J.R.; Physical Chemistry Laboratory Notebook, 2007 p. 22-23. Moore, L.G.; Physical Chemistry Laboratory Notebook, 2007 p. 18-19. Petty, A..; Physical Chemistry Laboratory Notebook, 2007 p. 24-25.